中文摘要：

circumstellar 日冕被建议在一个生长阶段期间解释一颗奇怪的夸克簇星，它能为理解思索的观察是必要的共生 X 光检查系统 4U 1700+24。在 supranuclear 密度的冷物质的状态仍然是争论的一种重要物质，并且充当一颗脉冲星的一颗奇怪的星的后果之一是表面上的自我界限现象，它使极其低团的紧缩的目标不可避免。原则上，在 blackbody 放射区域的 redshifted O VIII Ly- 排放线和变化能自然地被理解 4U 1700+24 是否是展览弯屈生长的一颗低团的夸克簇星。

英文摘要：

A circumstellar corona is proposed to explain a strange quark-cluster star during an accretion phase, which could be essential for understanding the observa- tions of the puzzling symbiotic X-ray system 4U 1700＋24. The state of cold matter at supranuclear density is still an important matter of debate, and one of the con- sequences of a strange star acting as a pulsar is the self-bound phenomenon on the surface, which makes extremely low-mass compact objects unavoidable. In principle, both the redshifted O VIII Ly-c~ emission line and the change in the blackbody radi- ation area could naturally be understood if 4U 1700＋24 is a low-mass quark-cluster star which exhibits wind accretion.